The evolution of EUI/HRI_EUV jet structure at 174 Å (top), the difference between Hα ±0.8 Å wing images (middle), and pseudo-Dopplergrams from five wavelength point GST/VIS images (bottom). They show a preexisting strand (a), a knot-like structure (b), multiple stripes ((b)–(d)), and a rapidly turning or bending structure ((e), (j), (o)) as well as sheath flows (arrows in (f)–(i) and (k)–(n)). The Dopplergrams show strong redshift components concentrated under the EUV jets.